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@ARTICLE{Tumasyan:600087,
      author       = {Tumasyan, Armen and others},
      collaboration = {{CMS Collaboration}},
      title        = {{F}irst measurement of the forward rapidity gap
                      distribution in p{P}b collisions at $\sqrt{s_\mathrm{{NN}}}$
                      = 8.16 {T}e{V}},
      journal      = {Physical review / D},
      volume       = {108},
      number       = {9},
      issn         = {2470-0010},
      address      = {Ridge, NY},
      publisher    = {American Physical Society},
      reportid     = {PUBDB-2023-07740, arXiv:2301.07630. CMS-HIN-18-019.
                      CERN-EP-2022-164},
      pages        = {092004},
      year         = {2023},
      abstract     = {For the first time at LHC energies, the forward rapidity
                      gap spectra from proton-lead collisions for both proton and
                      lead dissociation processes are presented. The analysis is
                      performed over 10.4 units of pseudorapidity at a
                      center-of-mass energy per nucleon pair of
                      $\sqrt{s_\mathrm{NN}}$ = 8.16 TeV, almost 300 times higher
                      than in previous measurements of diffractive production in
                      proton-nucleus collisions. For lead dissociation processes,
                      which correspond to the pomeron-lead event topology, the
                      EPOS-LHC generator predictions are a factor of two below the
                      data, but the model gives a reasonable description of the
                      rapidity gap spectrum shape. For the pomeron-proton
                      topology, the EPOS-LHC, QGSJET II, and HIJING predictions
                      are all at least a factor of five lower than the data. The
                      latter effect might be explained by a significant
                      contribution of ultra-peripheral photoproduction events
                      mimicking the signature of diffractive processes. These data
                      may be of significant help in understanding the high energy
                      limit of quantum chromodynamics and for modeling cosmic ray
                      air showers.},
      keywords     = {p nucleus: interaction (INSPIRE) / lead (INSPIRE) /
                      rapidity: gap (INSPIRE) / spectrum: gap (INSPIRE) /
                      diffraction: production (INSPIRE) / pomeron: exchange
                      (INSPIRE) / energy: high (INSPIRE) / showers: atmosphere
                      (INSPIRE) / rapidity dependence (INSPIRE) / topology
                      (INSPIRE) / diffraction: dissociation (INSPIRE) / cosmic
                      radiation (INSPIRE) / quantum chromodynamics (INSPIRE) /
                      photoproduction (INSPIRE) / peripheral (INSPIRE) / air
                      (INSPIRE) / CERN LHC Coll (INSPIRE) / signature (INSPIRE) /
                      experimental results (INSPIRE) / 8160 GeV-cms (INSPIRE)},
      cin          = {CMS},
      ddc          = {530},
      cid          = {I:(DE-H253)CMS-20120731},
      pnm          = {611 - Fundamental Particles and Forces (POF4-611) / DFG
                      project 390833306 - EXC 2121: Quantum Universe (390833306)},
      pid          = {G:(DE-HGF)POF4-611 / G:(GEPRIS)390833306},
      experiment   = {EXP:(DE-H253)LHC-Exp-CMS-20150101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2301.07630},
      howpublished = {arXiv:2301.07630},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2301.07630;\%\%$},
      UT           = {WOS:001123626500003},
      doi          = {10.1103/PhysRevD.108.092004},
      url          = {https://bib-pubdb1.desy.de/record/600087},
}